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Summer Solstice


Solstice comes from the Latin (sol, sun; sistit, stands). For several days before and after each solstice, the sun appears to stand still in the sky—that is, its noontime elevation does not seem to change.

Solstice, from the Latin for sun stands still, in astronomy, either of the two points on the ecliptic that lie midway between the equinoxes (separated from them by an angular distance of 90°).

At the solstices the sun's apparent position on the celestial sphere reaches its greatest distance above or below the celestial equator, about 23 1/2° of arc. At the time of summer solstice, about June 22, the sun is directly overhead at noon at the Tropic of Cancer.


In the northern hemisphere, the longest day of the year (near June 22) when the Sun is farthest north. In the southern hemisphere, winter and summer solstices are exchanged. The summer solstice marks the first day of the season of summer. The declination of the Sun on the (northern) summer solstice is known as the tropic of cancer (23° 27').

The summer solstice is the longest day of the year, respectively, in the sense that the length of time elapsed between sunrise and sunset on this day is a maximum for the year. Of course, daylight saving time means that the first Sunday in April has 23 hours and the last Sunday in October has 25 hours, but these human meddlings with the calendar and do not correspond to the actual number of daylight hours. In Chicago, there were15:02 hours of daylight on the summer solstice of June 21, 1999.

The above plots show how the date of the summer solstice shifts through the Gregorian calendar according to the insertion of leap years. The table below gives the universal time of the summer solstice. To convert to U. S. Eastern daylight saving time, subtract 4 hours, so the summer solstice occurs on June 21, 1998 at 10:00 a.m. EDT; June 21, 1999 at 15:47 (3:46 p.m.) EDT; and June 20, 2000 at 21:36 (9:36 p.m.) EDT.

Note that the times below were calculated using Summer Solstice in the Mathematica application package Scientific Astronomer, which is accurate to within only an hour or so, and in practice gives times that differ by up to 15 minutes from those computed by the U.S. Naval Observatory (which computes June 21, 1999 at 19:49 UT instead of 19:47 UT and June 21, 2000 at 01:48 UT instead of 01:36).

Date UT Date UT Date UT
06-21-1980 05:37 06-21-1990 15:36 06-21-2000 01:36
06-21-1981 11:25 06-21-1991 21:24 06-21-2001 07:24
06-21-1982 17:13 06-21-1992 03:13 06-21-2002 13:11
06-21-1983 23:00 06-21-1993 09:00 06-21-2003 18:59
06-21-1984 04:49 06-21-1994 14:48 06-21-2004 00:48
06-21-1985 10:37 06-21-1995 20:35 06-21-2005 06:36
06-21-1986 16:24 06-21-1996 02:24 06-21-2006 12:23
06-21-1987 22:12 06-21-1997 08:12 06-21-2007 18:11
06-21-1988 04:01 06-21-1998 14:00 06-21-2008 00:00
06-21-1989 09:48 06-21-1999 19:47 06-21-2009 05:47

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